Bianchi II with time varying constants. Self-similar approach
arXiv:0901.3827 · doi:10.1007/s10509-009-0050-6
Abstract
We study a perfect fluid Bianchi II models with time varying constants under the self-similarity approach. In the first of the studied model, we consider that only vary and The obtained solution is more general that the obtained one for the classical solution since it is valid for an equation of state while in the classical solution Taking into account the current observations, we conclude that must be a growing time function while is a positive decreasing function. In the second of the studied models we consider a variable speed of light (VSL). We obtain a similar solution as in the first model arriving to the conclusions that must be a growing time function if is a positive decreasing function.
10 pages. RevTeX4
References in corpus (25)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- The Cosmological Constant and Dark Energy
- Cosmological Constant - the Weight of the Vacuum
- The Case for a Positive Cosmological Lambda-term
- Discovery of a Supernova Explosion at Half the Age of the Universe and its Cosmological Implications
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae
- The fundamental constants and their variation: observational status and theoretical motivations
- Supernova Limits on the Cosmic Equation of State
- Constraints on Cosmological Models from Hubble Space Telescope Observations of High-z Supernovae
- A time varying speed of light as a solution to cosmological puzzles
- Superluminary Universe: A Possible Solution to the Initial Value Problem in Cosmology
- Cosmologies with Varying Light-Speed
- New varying speed of light theories
- Self-Similarity in General Relativity \endtitle
- Decaying Vacuum Energy and Deflationary Cosmology in Open and Closed Universes
- Geometrodynamics of Variable-Speed-of-Light Cosmologies
- Does a varying speed of light solve the cosmological problems?
- Measures of gravitational entropy I. Self-similar spacetimes
- The Weyl tensor in Spatially Homogeneous Cosmological Models
- Unusual Features of Varying Speed of Light Cosmologies
- Kinematic and Weyl singularities
- Bianchi I with variable and . Self-Similar approach
- About Bianchi I with VSL